SDO Observes Fast-Growing Sunspot
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- Visualizations by:
- Scott Wiessinger
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As magnetic fields on the sun rearrange and realign, dark spots known as sunspots can appear on its surface. Over the course of Feb. 19-20, 2013, scientists watched a giant sunspot form in under 48 hours. It has grown to over six Earth diameters across but its full extent is hard to judge since the spot lies on a sphere not a flat disk.
The spot quickly evolved into what's called a delta region, in which the lighter areas around the sunspot, the penumbra, exhibit magnetic fields that point in the opposite direction of those fields in the center, dark area. This is a fairly unstable configuration that scientists know can lead to eruptions of radiation on the sun called solar flares.

The bottom two black spots on the sun, known as sunspots, appeared quickly over the course of Feb. 19-20, 2013. These two sunspots are part of the same system and are over six Earths across. This image combines images from two instruments on NASA's Solar Dynamics Observatory (SDO): the Helioseismic and Magnetic Imager (HMI), which takes pictures in visible light that show sunspots and the Advanced Imaging Assembly (AIA), which took an image in the 304 angstrom wavelength showing the lower atmosphere of the sun, which is colorized in red.
Credit: NASA/SDO/AIA/HMI/Goddard Space Flight Center

Wider version of image. The bottom two black spots on the sun, known as sunspots, appeared quickly over the course of Feb. 19-20, 2013. These two sunspots are part of the same system and are over six Earths across. This image combines images from two instruments on NASA's Solar Dynamics Observatory (SDO): the Helioseismic and Magnetic Imager (HMI), which takes pictures in visible light that show sunspots and the Advanced Imaging Assembly (AIA), which took an image in the 304 angstrom wavelength showing the lower atmosphere of the sun, which is colorized in red.
Credit: NASA/SDO/AIA/HMI/Goddard Space Flight Center

Full Disk image at full SDO resolution. This image combines images from two instruments on NASA's Solar Dynamics Observatory (SDO): the Helioseismic and Magnetic Imager (HMI), which takes pictures in visible light that show sunspots and the Advanced Imaging Assembly (AIA), which took an image in the 304 angstrom wavelength showing the lower atmosphere of the sun, which is colorized in red.
Credit: NASA/SDO/AIA/HMI/Goddard Space Flight Center
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Credits
Please give credit for this item to:
NASA's Goddard Space Flight Center/SDO
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Animator
- Scott Wiessinger (KBR Wyle Services, LLC) [Lead]
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Writer
- Karen Fox (ADNET Systems, Inc.)
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Producer
- Scott Wiessinger (KBR Wyle Services, LLC)
Missions
This visualization is related to the following missions:Series
This visualization can be found in the following series:Tapes
This visualization originally appeared on the following tapes:-
2013 Heliophysics Breaking News
(ID: 2013021)
Tuesday, December 31, 2013 at 5:00AM
Produced by - Robert Crippen
Datasets used in this visualization
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SDO
ID: 168This dataset can be found at: http://sdo.gsfc.nasa.gov/
See all pages that use this dataset -
SDO SDO Continuum (Continuum)
ID: 674 -
SDO SDO Magnetogram (Magnetogram)
ID: 675 -
SDO AIA 304 (304 Filter)
ID: 677This dataset can be found at: http://jsoc.stanford.edu/
See all pages that use this dataset -
SDO AIA 171 (171 Filter)
ID: 680This dataset can be found at: http://jsoc.stanford.edu/
See all pages that use this dataset
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